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相关论文: A Systematic Survey of Moon-Forming Giant Impacts.…

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In the leading theory of lunar formation, known as the giant impact hypothesis, a collision between two planet-size objects resulted in a young Earth surrounded by a circumplanetary debris disk from which the Moon later accreted. The range…

地球与行星天体物理 · 物理学 2023-07-13 Miles Timpe , Christian Reinhardt , Thomas Meier , Joachim Stadel , Ben Moore

The hypothesis of lunar origin by a single giant impact can explain some aspects of the Earth-Moon system. However, it is difficult to reconcile giant impact models with the compositional similarity of the Earth and Moon without violating…

地球与行星天体物理 · 物理学 2019-03-07 Raluca Rufu , Oded Aharonson , Hagai B. Perets

The multiple impact hypothesis proposes that the Moon formed through a series of smaller collisions, rather than a single giant impact. This study advances our understanding of this hypothesis, as well as moon collisions in other contexts,…

地球与行星天体物理 · 物理学 2024-11-14 Uri Malamud , Hagai Perets

The giant impact hypothesis is the dominant theory of how the Earth-Moon system was formed. Models have been created that can produce a disk of debris with the proper mass and composition to create our Moon. Models have also been created…

地球与行星天体物理 · 物理学 2013-07-29 Justin C. Eiland , Travis C. Salzillo , Brett H. Hokr , Justin L. Highland , Bryant M. Wyatt

Giant impacts refer to collisions between two objects each of which is massive enough to be considered at least a planetary embryo. The putative collision suffered by the proto-Earth that created the Moon is a prime example, though most…

地球与行星天体物理 · 物理学 2016-04-13 Mark C. Wyatt , Alan P. Jackson

The Moon is believed to have formed in the aftermath of a giant impact between a planetary mass body and the proto-Earth. In a typical giant impact scenario, a disk of vapor, liquid, and solid debris forms around the proto-Earth and--after…

地球与行星天体物理 · 物理学 2020-11-11 P. D. Mullen , C. F. Gammie

The Earth-Moon system is suggested to have formed through a single giant collision, in which the Moon accreted from the impact-generated debris disk. However, such giant impacts are rare, and during its evolution the Earth experienced many…

地球与行星天体物理 · 物理学 2018-08-01 Robert I. Citron , Hagai B. Perets , Oded Aharonson

In order to examine the ``giant impact hypothesis'' for the Moon formation, we run the first grid-based, high-resolution hydrodynamic simulations for an impact between proto-Earth and a proto-planet. The spatial resolution for the…

天体物理学 · 物理学 2009-11-11 Keiichi Wada , Eiichiro Kokubo , Junichiro Makino

According to the giant impact theory, the Moon formed by accreting the circum-terrestrial debris disk produced by Theia colliding with the proto-Earth. The giant impact theory can explain most of the properties of the Earth-Moon system,…

地球与行星天体物理 · 物理学 2025-05-15 Wenshuai Liu

We investigate the possibility that the Moon's formation impact was triggered by an early dynamical instability of the giant planets. We consider the well-studied "jumping Jupiter" hypothesis for the solar system's instability, where…

地球与行星天体物理 · 物理学 2021-08-11 Sandro R. DeSouza , Fernando Roig , David Nesvorný

We simulate the hypothesised collision between the proto-Earth and a Mars-sized impactor that created the Moon. Amongst the resulting debris disk in some impacts, we find a self-gravitating clump of material. It is roughly the mass of the…

地球与行星天体物理 · 物理学 2020-12-09 Sergio Ruiz-Bonilla , Vincent R. Eke , Jacob A. Kegerreis , Richard J. Massey , Luis F. A. Teodoro

The Moon is generally thought to have formed from the debris ejected by the impact of a planet-sized object with the proto-Earth towards the end of planetary accretion. Modeling of the impact process predicts that the lunar material was…

地球与行星天体物理 · 物理学 2016-04-19 Kaveh Pahlevan , Alessandro Morbidelli

Giant impacts dominate the final stages of terrestrial planet formation and set the configuration and compositions of the final system of planets. A giant impact is believed to be responsible for the formation of Earth's Moon, but the…

地球与行星天体物理 · 物理学 2020-02-05 Philip J Carter , Simon J Lock , Sarah T Stewart

During the last stages of the terrestrial planet formation, planets grow mainly through giant-impacts with large planetary embryos. The Earth's Moon was suggested to form through one of these impacts. However, since the proto-Earth has…

地球与行星天体物理 · 物理学 2018-07-11 Uri Malamud , Hagai B. Perets , Christoph Schafer , Christoph Burger

The proposed multi-impact model explains the formation of the Moon, Charon, and binary asteroids without invoking catastrophic cosmic events. The main elements of the new model are as follows: a. A primordial, low-mass proto-satellite disk…

地球与行星天体物理 · 物理学 2025-12-30 Nick Gorkavyi

Most of the properties of the Earth-Moon system can be explained by a collision between a planetary embryo and the growing Earth late in the accretion process. Simulations show that most of the material that eventually aggregates to form…

地球与行星天体物理 · 物理学 2015-06-24 Alessandra Mastrobuono-Battisti , Hagai B. Perets , Sean N. Raymond

Planets are expected to conclude their growth through a series of giant impacts: energetic, global events that significantly alter planetary composition and evolution. Computer models and theory have elucidated the diverse outcomes of giant…

地球与行星天体物理 · 物理学 2023-12-27 Travis S. J. Gabriel , Saverio Cambioni

The leading theory for the origin of the Moon is the giant impact hypothesis, in which the Moon was formed out of the debris left over from the collision of a Mars-sized body with the Earth. Soon after its formation, the orbit of the Moon…

科普物理 · 物理学 2015-03-11 Emil Noordeh , Patrick Hall , Matija Cuk

Exomoons orbiting terrestrial or super-terrestrial exoplanets have not yet been discovered; their possible existence and properties are therefore still an unresolved question. Here we explore the collisional formation of exomoons through…

地球与行星天体物理 · 物理学 2020-01-29 Uri Malamud , Hagai B. Perets , Christoph Schaefer , Christoph Burger

In the canonical model of Moon formation, a Mars-sized protoplanet "Theia" collides with proto-Earth at close to their mutual escape velocity $v_{\rm esc}$ and a common impact angle 45{\deg}. The "graze-and-merge" collision strands a…

地球与行星天体物理 · 物理学 2021-10-04 Erik Asphaug , Alexandre Emsenhuber , Saverio Cambioni , Travis S. J. Gabriel , Stephen R. Schwartz
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